Subject: MM#009 Default Target" --><br>
<span id="date"><dfn>Date</dfn>: Tue, 21 Jul 2020 13:10:36 +0100</span><br /><br>
</address> <pre> </pre> Dear Collaborators,
<br />Solar activity remains at an extremely low level. The leading polarity
footpoints of the target EUV coronal-loop region have rotated over the
South East limb onto the visible disk. This region shows a reasonably
sized sunspot and, although it is too close to the limb to be certain,
it appears to have a mature and symmetric penumbra. This region was the
source of a partly occulted A-class flare since the last email (an A2.8
on 20-Jul-2020 at 23:30 UT). Low B-class activity is possible over the
next 24-hour period as this region's trailing polarity flux rotates on disk.
<br />The approximate position of this region on 21-Jul-2020 at 12:00 UT is:
<br />S21E90 , ( -881&quot;, -337&quot; )
<br />See <a href="http://www.SolarMonitor.org">http://www.SolarMonitor.org</a> for images and
<a href="http://solar.physics.montana.edu/max_millennium/ops/observing.shtml">http://solar.physics.montana.edu/max_millennium/ops/observing.shtml</a>
for a description of the current Max Millennium Observing Plan. <br />Regards,
<br />Shaun Bloomfield (Northumbria University)
<span id="received"><dfn>Received on</dfn> Tue Jul 21 2020 - 06:10:47 MDT</span>
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